Gravitational question ( calculus )

AI Thread Summary
The discussion focuses on calculating the time of collision (T) between two point masses (M1 and M2) due to gravitational attraction, starting from an initial separation (r0). The user attempts to derive T using calculus and the conservation of energy, integrating to find the displacement and velocity as the masses approach each other. They express concerns about the complexity of the integration process and whether their approach is conceptually sound. The user seeks assistance to confirm their method and resolve any potential errors in their calculations. The thread highlights the challenges of applying calculus to gravitational problems in classical mechanics.
peterpang1994
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Homework Statement


2 point mass M1 and M2 . Their separation is r0. They are released at rest at t=0. Find the time of collision (T)of them due to gravitational attraction in terms of M1, M2 , G and r0.

Homework Equations


F=ma
∫a(dt)2 = s (a is acceleration, s is displacement)
x0=(M2/(M1 + M2))r0 ( x is the position of center of mass respect to M1 )
F=-GM1M2/r2

The Attempt at a Solution


I used ∫a(dt)2 = s and make it becomes dt=(v/a)ds. As they should collide at the center of mass, the displacement of M1 should be equals to x. Therefore,
T=∫(v/a)dx
sup x=(M2/(M1 + M2))r , let (M2/(M1 + M2)) = R
x=Rr
dx=Rdr
T=R∫(v/a)dr (from r=r0 to r=0)
By law of conservation of energy,
(1/2)M1v2 = GM1M2(1/r - 1/r0)
v=√(2GM2(1/r - 1/r0))
a=GM2/r2
∴T=R∫√(2GM2(1/r - 1/r0)) / (GM2/r2) dr
After some calculation, I got
T=R√(2/(GM2r02))∫r2√(1/r - 1/r0)dr (from r=r0 to r=0)
I found that integration is very difficult. I wonder whether I get the correct direction or having conceptional and calculating error. I just hope that any help can be given. Thanks a lot.

Homework Statement


Homework Equations


The Attempt at a Solution

 
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